Boulby International Subsurface Astrobiology Laboratory (BISAL) Charles Cockell, Sean Paling, David Pybus, David McLuckie et al.

Slides:



Advertisements
Similar presentations
I3/CA Europlanet - EC Contract EUROPLANET in FP-7 Tentative overall structure of Europlanet in FP7 and further Preparations.
Advertisements

The Traveling Exhibit Science Background Part D: Search for Life prepared by Dr. Cherilynn Morrow for the Space Science Institute Boulder, CO.
Space Exploration Mars Rovers, Apollo program, Voyager satellites, and SETI All Presented by the Peter C Period: 2 (two) As in 1+1=2 Or 2x1=2 ®
1 Partnering Presented at JUSTSAP/PISCES 2008 Collaboration with Colorado School of Mines.
An Introduction to the Boulby Underground Labs
Underground Facilities Stub 2 Stub 2a,3 ‘H’ Area JIF Area The underground research facilities have evolved since dark matter studies began at Boulby. There.
Geobiology in Space Exploration An ESA/Global Topical Team.
First Marine Board Forum – 15 May Oostende Marine Data Challenges: from Observation to Information From observation to data.
Background Measurements and Boulby for JRA1 Tim Lawson University of Sheffield IAP, Paris, 14 th February 2006.
Thursday, October 20 4:00-8:00pm University of Colorado (room to be announced). Please register for this free workshop now at
Lunar Advanced Science and Exploration Research: Partnership in Science and Exploration Michael J. Wargo, Sc.D. Chief Lunar Scientist for Exploration Systems.
Copyright (c) John Y. Cheung, 2002 ECE Recruiting,ppt Slide 1 What is an Electrical and Computer Engineer?
Beyond Tang: The Hidden Benefits of the Space Program Dr. Nadine G. Barlow Dept. Physics and Astronomy Northern Arizona University Flagstaff, AZ.
14 July 2000TWIST George Brett NLANR Distributed Applications Support Team (NCSA/UIUC)
The neutrons detection involves the use of gadolinium which has the largest thermal neutron capture cross section ever observed. The neutron capture on.
Office of Science Office of Biological and Environmental Research J Michael Kuperberg, Ph.D. Dan Stover, Ph.D. Terrestrial Ecosystem Science AmeriFlux.
SWCX and the production of X-rays SWCX produces X-rays when heavy ions in the solar wind interact with neutrals in the Earth’s exosphere, cometary nebulae,
CAISU Workshop, November 5, 2004 Canadian Expertise Relevant to Exploration David Kendall Director General Space Science Program CAISU Workshop, CSA Headquarters,
The Traveling Exhibit Electronic Guided Tour 1. Key Partners Principal Funders: 2.
Low-Background Activation Analysis NAA for ultrapure materials analysis Richard M. Lindstrom Analytical Chemistry Division National Institute of Standards.
The Edinburgh Research Partnership in Engineering and Mathematics Heriot-Watt University EH14 4AS University of Edinburgh EH9 3LA ECOSSE.
High Altitude Scientific Ballooning (Near Space Engineering)
Mars Exploration Directorate National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California.
What is Oceanography?. Marine Science Or oceanography is the study of the oceans, how they are formed, its associated life forms, the coastal interactions,
Understanding the Mars Mission and soil studies by using the web A Web project.
Intelligent Robotics Group NASA Ames Research Center Intelligent Robotics Group NASA Ames Research Center Planning for the Mapping and Exploration of Human.
International ScientificThematic Network for Environmental Technologies ENVITECH-Net.
Status and Plans The Boulby Underground Science Facility (UK)
 Kalgoolie, Australia  Salt Evaporation Ponds.
Building Science Capacity using Seismology Michelle Grobbelaar.
Science Investigation Life in the Atacama 2004 Science & Technology Workshop Nathalie A. Cabrol NASA Ames.
John Womersley John Womersley Director, Science Programmes Science and Technology Facilities Council Technology Gateway Centres.
Space Program Benefits US Space Program has been around since 1958 US Space Program has been around since 1958 Technology developed for space program has.
Mars Exploration Rovers (MER) Entry, Descent, Landing, and Deployment.
VdG:ISME - July Vasco da Gama In Situ Mars Explorer.
1 Quality Assurance Office Supplier Outreach & Process Control For NASA’s Space Programs (Earth Science, Space Science, and Biological and Physical Research)
1. Overview About Washington University / Planetary Data Systems Geosciences Node Initial and continued interactions in China NASA-CNSA Bilateral (July.
1 Enviromatics Environmental sampling Environmental sampling Вонр. проф. д-р Александар Маркоски Технички факултет – Битола 2008 год.
Mars Geochemistry and Future Experiment Needs Mark A. Bullock August 7, 2002.
Curiosity Rover.
Europlanet RI A network for all planetary scientists A service to the community Manuel Grande Scientific Dissemination Coordinator EC grant agreement no.
RASC-AL 2010 Topics. TECHNOLOGY-ENABLED HUMAN MARS MISSION NASA is interested in eventual human mission to the Martian surface. Current Mars design reference.
Boulby Laboratory (UK) Middlesborough Whitby Staithes York.
Unit 6 Lesson 1 Explanation. In 2004, President Bush set the following goal for the NASA constellation program, “this vision… is a sustainable and affordable.
1 Atmospheric Radiation – Lecture 17 PHY Lecture 17 Satellite instruments and missions.
Semantic Metadata for Scientific Data Access and Management Richard M. Keller, Ph.D. Group Lead for Information Sharing & Integration Intelligent Systems.
Internet2 Applications Group: Renater Group Presentation T. Charles Yun Internet2 Program Manager, Applications Group 30 October 2001.
Enabling Capabilities A Robotic Field Geologist Access to a site mapped from orbit Long life, mobility, capability to explore a local region Remote sensing.
Life on Mars? 17 February Are we alone? Life arose quickly on Earth, around 4 billion years ago Star formation makes planets, too: they should be.
DEPARTMENT OF PHYSICS AND ASTRONOMY X-ray Astronomy and Space Instrumentation I3 Meeting, December 2004 Integrating Space Radiation Sensing Infrastructures.
Colorado Space Grant Symposium 2011 Meeting Colorado School of Mines Affiliate.
Dr Annika Lohstroh (RDI Theme chair) on behalf of the RDI steering committee Department of Physics, University of Surrey, UK South East Physics Network.
Curiosity Rover By Abby Bradshaw and Paige Taylor.
National Aeronautics and Space Administration Astromaterials Research and Exploration Science 1 NASA—Johnson Space Center Astromaterials Research and Exploration.
Lunar Surface Atmosphere Spectrometer (LSAS) Objectives: The instrument LSAS is designed to study the composition and structure of the Lunar atmosphere.
Deep Science at Boulby Underground Laboratory:
Improving Canadian Capacity for Predicting the Impacts of Natural and Human Disturbances on Boreal Water Resources Canadian Aquatic Laboratory for Interdiscplinary.
Jacob Bleacher: Goddard Space Flight Center 2016 Humans to Mars Summit Collaborators: Remote, In Situ & Syncrotron Studies for Science and Exploration.
Deep Science at Boulby Underground Laboratory:
Space Robot APARNA .K.P SITHARA.P.SUNDARAN VJEC.
1.1: Comparing Rocky Planets
Project and Workshop Objectives
Exploration of Subsurface Mars’ Geology and Water
Goddard Contractor Association
Beyond Tang: The Hidden Benefits of the Space Program
Challenger Learning Center of Colorado
Design 6 Classes 4th Quarter Lunar/Mars Rover Science Project
Life on Mars? 4 October 2017.
Life on Mars? 20 February 2018.
Public Engagement Lead LRO and SAM
Presentation transcript:

Boulby International Subsurface Astrobiology Laboratory (BISAL) Charles Cockell, Sean Paling, David Pybus, David McLuckie et al.

Boulby Mine A working potash and rock-salt mine on the North East of England. Operated by Cleveland Potash Ltd. Major local employer - ~1000 direct and 4000 indirect employment. Middlesborough Whitby Staithes York Potash `View from Staithes Deepest mine in Britain – 1100m deep (2805mwe) – Cosmic ray muon flux reduced by 10 6

ZEPLIN-III DRIFT-II SKY ‘JIF’ Science Facilities (opened 2003). ‘Palmer Lab’: a 100+m, fully equipped underground lab. Power, internet and telephone communications, lifting, air conditioning / filtration, clean room. ‘John Barton’ surface facility: Workshop, facility monitoring, office and administration, PPE, storage, chemistry lab, changing rooms. Boulby Science facilities A QUIET place in the Universe

The mission of the UK Centre for Astrobiology is to advance our understanding of molecules and life in extreme environments on the Earth and beyond. It does this by a combination of theoretical, laboratory, field and mission approaches. We apply this knowledge to improving the quality of life on Earth and developing space exploration as two mutually enhancing objectives.

Research Affiliate Nodes (RANs)

Astrobiology/geomicrobiology science at Boulby:  Life in the deep subsurface  Life in deep salts  Deep cycling of elements  Geobiology, Geochemistry and Geophysics of deep subsurface environments  Life at below surface background radiation  Life in extreme environments/life elsewhere

The search for life on Mars Mars is covered in salts We need to know about life in anaerobic salty environments to be able to explore Mars Seeps of salty water on Mars McEwan et al. (2011) Science 333, 740

We already know that Boulby is scientifically interesting for the study of life Study of shales in the interior of Boulby cliffs revealed:  New insights into how microbes interact with minerals.  New types of microbes associated with shales  Links between microbes and coastal erosion. Work supported by CPL The study of the link between microbes and coastal erosion Cockell CS, Pybus D, Olsson-Francis K, Kelly L, Petley D, Rosser N, Howard K, Mosselmans F Molecular Characterization and Geological Microenvironment of a Microbial Community Inhabiting Weathered Receding Shale Cliffs. Microbial Ecology 61, This work was reported in the STFC Diamond annual report.

Boulby ‘Palmer Lab’ Stub A Low Background Lab AB DRIFT-I store Mess Gas/fire sensor control Entrance corridor gas sensors ZEPLIN-II Germanium Detector / castle Workshop Store DRIFT-II Control room Class 10,000 Clean room Class 1,000 Clean room ~70m ~20m ~6m 5m Materials End Store Main Hall Clean off area People entrance Materials entrance ZEPLIN-III SKY

Existing Deep Subsurface Laboratories - The International Context LaboratoryDepthSubstrate Boulby International Subsurface Astrobiology Laboratory, Yorkshire, UK 1.1 kmPermian salt Sudbury Neutrino Observatory, Ontario 2.07 kmNorite granite Laboratoire Souterrain de Modane, France 1.75 kmSchistes lustres Gran Sasso National Laboratory, Italy 1.4 kmDolomite and limestone Äspö Hard Rock Laboratory, Sweeden 500 mDorite, granite and greenstone HADES Laboratory, Belgium224 mBoom clay BISAL will be: -First permanent subsurface astrobiology laboratory -First permanent subsurface microbiology laboratory in salts -One of the world’s deepest permanent microbiology laboratories

Caves on Mars Boulby as a Mars and Moon analogue environment Subsurface environments teach us how to explore (and exploit) caves on the moon and Mars

Subsurface environments on Mars provide protection from: 1) UV radiation 2) Ionising radiation on the surface of Mars - and might therefore be good places to search for life in the subsurface of Mars and to understand past geochemical processes in general To explore these environments we need to know more about:  Life in the deep subsurface  How to study life in the deep subsurface  What technologies we might use in the subsurface Boulby provides the ideal environment to develop methods and approaches for the exploration of Mars.

Boulby surface Mine The mine is to be used to test rovers for the subsurface exploration of the Moon and Mars Rovers MINAR – Mining and Analogue Research

Boulby as a Mars Analog – the NASA link Lim et al 2010 Lim et al 2010, Planetary Space Science

SCIENCE SUPPORT TOOLS: Mission architectures used at Pavilion Lake would be transferred to Boulby Fiber Optic Tether: Approx 200 meters of tether connect the submersible to the surface control vessel. Surface Control Vessel: The surface vessel has a fiber optic to Ethernet converter similar to the hardware used on the DeepWorker. Two way “hardwire voice communication are available as well as real time video from the submersible’s main camera. This Ethernet data can then be broadcast wirelessly using the existing network system to the Science Back-Room. CapCom Navigator StenoDriver WinFrog Stenographer Tools Through Water Comms Topside Deep Worker Pilot Surface Data System

Team NASA – Coming to Boulby Team members have supported every major NASA field deployment including the Pavilion Lake Research Project, NEEMO, DRATs, RESOLVE and the Haughton Mars Project. Science, engineering and operations expertise represented NASA and US science participation in Boulby Mine activities will be coordinated by Darlene Lim at NASA Ames

Boulby and Instrumentation for Earth and Space Exploration  A major challenge in space exploration is miniaturising instrumentation because of the mass and energy cost of transporting materials into space. This is true for both robotic and human exploration. BISAL will allow us to test life detection and general analytical technologies (e.g. IR and Raman spectroscopy, portable XRD and XRF etc) that could be used in space exploration missions and applied to Earth-based problems such as mining safety. BISAL will provide a new capability to develop instrumentation for extreme environments on the Earth and in space

Meetings How is this to be done?..by a three day workshop “Boulby/BISAL as an extraterrestrial analogue” April 22-24, 2013 Two days of visiting the mine (April 22-23) with discussions on the architecture of a Mars/Moon analogue programme followed by One day workshop (April 24): ‘From Outer Space to Mining’ -Focused on how we can take space technologies (such as STFC-funded technologies) and apply them to mining safety and mineral extraction

Summary of BISAL What is the BISAL?  A Palmer-lab based facility to allow for the study of life in extreme subsurface environments, particularly salts.  A facility to assist in the development of instrumentation for the exploration of extreme terrestrial and extraterrestrial environments and its application to solving Earth-based problems, particularly in mining safety, mineral exploitation and geostorage  A facility to ignite international excitement for astrobiology and the study of life in extreme environments.  Linked to the NASA Astrobiology Institute through the UK Centre for Astrobiology at Edinburgh.

How will BISAL work? Practicalities  Establishment of basic clean sample collection, culturing facilities, sample analysis and DNA extraction in the BISAL lab in the existing Palmer lab.  Site visits for work several times a year for 2-3 days each time depending on interest and level of involvement (students, postdocs etc). Logistics  Science coordination and work overseen by UKCA, the UK Centre for Astrobiology, based at the University of Edinburgh in co-ordination with Boulby/CPL.  Site logistics in co-ordination with Sean Paling, STFC.